Phase shift sequences for an adding interferometer

doi:10.1111/j.1365-2966.2008.14194.x

2009-02-21

Hyland, Peter *

Follin, Brent

Emory F. Bunn

DOI：10.1111/j.1365-2966.2008.14194.x

原文链接

查看原文

摘要

En 中文

Cosmic microwave background (CMB) polarimetry has the potential to provide revolutionary advances in cosmology. Future experiments to detect the very weak B-mode signal in CMB polarization maps will require unprecedented sensitivity and control of systematic errors. Bolometric interferometry may provide a way to achieve these goals. In a bolometric interferometer (or other adding interferometer), phase shift sequences are applied to the inputs in order to recover the visibilities. Noise is minimized when the phase shift sequences corresponding to all visibilities are orthogonal. We present a systematic method for finding sequences that produce this orthogonality, approximately minimizing both the length of the time sequence and the number of discrete phase shift values required. When some baselines are geometrically equivalent, we can choose sequences that read out those baselines simultaneously, which has been shown to improve the signal-to-noise ratio.

Keyword:

techniques: interferometric

techniques: polarimetric

cosmic microwave background

AI总结

对已上传原文的论文进行重点信息的提取，主要内容包括：简要概述、研究摘要、背景介绍、关键亮点、图文解析、展望与总结。

期刊

Monthly Notices of the Royal Astronomical Society

IF:

4.8

论文数:

7.0W

被引数:

25.0W

机构

university of wisconsin madison

学者数:

3.8W

论文数: 2.9W

被引数: 53

University of Wisconsin System

学者数:

6.7W

论文数: 5.8W

被引数: 382

引用论文

Evolution of the Large Scale Circulation, Cloud Structure and Regional Water Cycle Associated with the South China Sea Monsoon during May-June, 1998.

Journal of the Meteorological Society of Japan. Ser. II

IF0

2002-01-01

OAAI

K.-M LAU; Xiaofan LI; H.T WU

Degree Angular Scale Interferometer 3 year cosmic microwave background polarization results

ASTROPHYSICAL JOURNAL

IF5.4

2005-05-01

171

OAAI

Leitch, EM; Kovac, JM; Halverson, NW; Carlstrom, JE; Pryke, C; Smith, MWE

Possible Causes of Anomalies in Seasonal Mean Circulation Patterns during the 1982–83 El Niño Event

Journal of the Atmospheric Sciences

IF0

1985-04-01

OAAI

C. J. Kok; J. D. Opsteegh

The Einstein polarization interferometer for cosmology (EPIC) and the millimeter-wave bolometric interferometer (MBI)用于宇宙学的爱因斯坦偏振干涉仪 (EPIC) 和毫米波辐射热干涉仪 (MBI)

NEW ASTRONOMY REVIEWS

IF26.8

2006-12-01

OAAI

Timbie, P. T.; Tucker, G. S.; Ade, P. A. R.; Ali, S.; Bierman, E.; Bunn, E. F.; Calderon, C.; Gault, A. C.; Hyland, P. O.; Keating, B. G.; Kim, J.; Korotkov, A.; Malu, S. S.; Mauskopf, P.; Murphy, J. A.; O'Sullivan, C.; Piccirillo, L.; Wandelt, B. D.

Meine Myelogenetische Hirnlehre

IF0

1927-01-01

PREAI

Paul Flechsig

The BRAIN CMB polarization experiment

NEW ASTRONOMY REVIEWS

IF26.8

2007-03-01

OAAI

Polenta, G.; Ade, P. A. R.; Bartlett, J.; Breelle, E.; Conversi, L.; de Bernardis, P.; Dufour, C.; Gervasi, M.; Giard, M.; Giordano, C.; Giraud-Heraud, Y.; Maffei, B.; Masi, S.; Nati, F.; Orlando, A.; Peterzen, S.; Piacentini, F.; Piat, M.; Piccirillo, L.; Pisano, G.; Pons, R.; Rosset, C.; Savini, G.; Sironi, G.; Tartari, A.; Veneziani, M.; Zannoni, M.

Experimental investigation and calculation of the binary (AgNO 3 + KNO 3 ) phase diagram

The Journal of Chemical Thermodynamics

IF0

2015-02-01

PREAI

D. Boa; D. Hellali; D. Licbarski; M. Tizzotti; H. Zamali; C. Favotto; P. Benigni; J. Rogez

Carcinoma of the Lower Uterine Segment (LUS): Clinicopathological Characteristics and Association with Lynch Syndrome

Current Genomics

IF0

2011-03-01

OAAI

Kenta Masuda; Kouji Banno; Megumi Yanokura; Yusuke Kobayashi; Iori Kisu; Arisa Ueki; Asuka Ono; Hiroyuki Nomura; Akira Hirasawa; Nobuyuki Susumu; Daisuke Aoki

Sensitivity of a bolometric interferometer to the cosmic microwave backgroud power spectrum

ASTRONOMY & ASTROPHYSICS

IF5.8

2008-10-07

OAAI

Hamilton, J. -Ch.; Charlassier, R.; Cressiot, C.; Kaplan, J.; Piat, M.; Rosset, C.

没有更多内容